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FWF National Research Program (NFN): Pathways to Habitability (PatH)

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Home | path.univie.ac.at Reviews
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FWF National Research Program (NFN): Pathways to Habitability (PatH)
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1 pathways to habitability
2 meetings
3 publications
4 committee
5 acknowledgements
6 overview
7 print
8 email
9 details
10 main menu
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pathways to habitability,meetings,publications,committee,acknowledgements,overview,print,email,details,main menu,internal,sp2 disks,sp3 water,sp4 stars,sp5 sun,sp6 magnetospheres,sp7 atmospheres,sp8 binary stars,login form,username,remember me,conferences
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Home | path.univie.ac.at Reviews

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FWF National Research Program (NFN): Pathways to Habitability (PatH)

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1

Publications 2013

http://path.univie.ac.at/index.php/publications/publications-2013

Onclick="window.open(this.href,'win2','status=no,toolbar=no,scrollbars=yes,titlebar=no,menubar=no,resizable=yes,width=640,height=480,directories=no,location=no'); return false;" rel="nofollow". Last Updated: 10 July 2015. Sorted by article title). Characterizing Exoplanets in the Visible and Infrared: a Spectrometer Concept for the EChO Space Mission. J Astron. Instrumentation 2, id. 1350004. Eggl, S., Pilat-Lohinger, E., Funk, B., Georgakarakos, N., Haghighipour, N. (2013). IAU Symposium 302 (in press).

2

Meetings 2016

http://path.univie.ac.at/index.php/meetings/meetings-2016

Onclick="window.open(this.href,'win2','status=no,toolbar=no,scrollbars=yes,titlebar=no,menubar=no,resizable=yes,width=640,height=480,directories=no,location=no'); return false;" rel="nofollow". Last Updated: 04 October 2016. Sorted by date in reverse order). R Dvorak, B. Loibnegger, T. I. Maindl (talk). Comparison of impact scenaria in the Solar System. Stardust final conference of asteroids and space debris, 31 Oct - 4 Nov, 2016, ESA/ESTEC, Noordwijk, The Netherlands. Realistic modeling of water tranfer...

3

Publications 2015

http://path.univie.ac.at/index.php/publications/publications-2015

Onclick="window.open(this.href,'win2','status=no,toolbar=no,scrollbars=yes,titlebar=no,menubar=no,resizable=yes,width=640,height=480,directories=no,location=no'); return false;" rel="nofollow". Last Updated: 07 October 2016. Sorted by article title). Bancelin, D., Pilat-Lohinger, E., Eggl, S., Maindl, T. I., Schäfer, C., Speith, R., Dvorak, R. (2015). Asteroid flux towards circumprimary habitable zones in binary star systems: I. Statistical Overview. A&A, 581, A46. MNRAS, 448, 3797. A&A, 577, A122, 13.

4

Committee

http://path.univie.ac.at/index.php/committee

Steering and Advisory Committee. Onclick="window.open(this.href,'win2','status=no,toolbar=no,scrollbars=yes,titlebar=no,menubar=no,resizable=yes,width=640,height=480,directories=no,location=no'); return false;" rel="nofollow". Last Updated: 24 March 2014. Prof Dr. Douglas N.C. Lin. Professor of Astronomy and Astrophysics. Astronomy and Astrophysics Department. Office: 337 Interdisciplinary Sciences. University of California, Santa Cruz, USA. Santa Cruz, CA 95064. Prof Dr. Rickard Lundin. CNRS/UPS UMR 814...

5

Meetings 2013

http://path.univie.ac.at/index.php/meetings/meetings-2013

Onclick="window.open(this.href,'win2','status=no,toolbar=no,scrollbars=yes,titlebar=no,menubar=no,resizable=yes,width=640,height=480,directories=no,location=no'); return false;" rel="nofollow". Last Updated: 27 May 2015. Sorted by date in reverse order). Atmospheric expansion and mass loss of XUV heated hydrogen-dominated exoplanets. ISSI Team Meeting "Characterizing stellar and exoplanetary environments via observations and advance, December 2013, Bern/Switzerland. RDvorak, (Invited Talk). Z Sándor (Con...

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habitability.univie.ac.at habitability.univie.ac.at

The Astrophysics of Planetary Habitability

https://habitability.univie.ac.at/home

The Astrophysics of Planetary Habitability Home. With a continuously increasing number of discovered exoplanets, research is shifting from pure detection to characterization of planets. The rapidly improving quality of observing tools and the success of space-based observations of exoplanets are driving detection and characterization toward ever smaller planets; several rocky planets have already been detected in or near habitable zones around their host stars. Key issues include, among others. The effec...

habitability.univie.ac.at habitability.univie.ac.at

The Astrophysics of Planetary Habitability

http://habitability.univie.ac.at/sitemap

The Astrophysics of Planetary Habitability Sitemap. How to get there. The Astrophysics of Planetary Habitability Universitätsring 1 1010 Wien.

habitability.univie.ac.at habitability.univie.ac.at

The Astrophysics of Planetary Habitability

http://habitability.univie.ac.at/important-dates

The Astrophysics of Planetary Habitability Important Dates. Please note these important dates and deadlines (updated):. Deadline for abstract submission. Deadline for early registration. Registration fee 200/100 Euro for regular/student). Deadline for late registration. Registration fee 250/150 Euro for regular/student). On-site registration desk will be available at these times:. Monday (8 February 2016) beginning from 12:00 pm. Tuesday and Wednesday (9/10 February 2016) from 8:30 am.

habitability.univie.ac.at habitability.univie.ac.at

The Astrophysics of Planetary Habitability

http://habitability.univie.ac.at/home/photographs

The Astrophysics of Planetary Habitability Photographs. Click on the image to download a selection of photographs taken during the conference. There are 115 images in this compressed ZIP archive (file size 477 MB). The Astrophysics of Planetary Habitability Universitätsring 1 1010 Wien.

habitability.univie.ac.at habitability.univie.ac.at

The Astrophysics of Planetary Habitability

http://habitability.univie.ac.at/impressum

The Astrophysics of Planetary Habitability Impressum. The Astrophysics of Planetary Habitability Universitätsring 1 1010 Wien.

habitability.univie.ac.at habitability.univie.ac.at

The Astrophysics of Planetary Habitability

http://habitability.univie.ac.at/program

The Astrophysics of Planetary Habitability Program. The program runs from Monday (February 8) 1 pm until Friday (February 12) 1 pm. On Monday evening there will be a visit to the monastery at Klosterneuburg, followed by a reception at the observatory of the University of Vienna. On Thursday afternoon we will visit the world famous meteorite collection of the Natural History Museum of Vienna, followed by a conference dinner at the town hall (Rathaus) of Vienna. V Meadows (Univ. Washington). The effects of...

habitability.univie.ac.at habitability.univie.ac.at

The Astrophysics of Planetary Habitability

http://habitability.univie.ac.at/venue

The Astrophysics of Planetary Habitability Venue. How to get there. University of Vienna, Main Building. The fully disabled-accessible Assembly Hall, which also features a modern info-center, leads to the green Arcade Courtyard, where in the warm season an open air cafeteria lures those in need of a moment of repose. Busts and statues under the arcades keep the memory of renowned university professors alive. The Astrophysics of Planetary Habitability Universitätsring 1 1010 Wien.

habitability.univie.ac.at habitability.univie.ac.at

The Astrophysics of Planetary Habitability

http://habitability.univie.ac.at/home/loc

The Astrophysics of Planetary Habitability LOC. The Astrophysics of Planetary Habitability Universitätsring 1 1010 Wien.

habitability.univie.ac.at habitability.univie.ac.at

The Astrophysics of Planetary Habitability

http://habitability.univie.ac.at/participants

The Astrophysics of Planetary Habitability Participants. List of confirmed participants (alphabetical order). Last update: 2016 Feb 01. Total number of participants: 142. List of confirmed participants. Alvarado Gomez Julian David. The Astrophysics of Planetary Habitability Universitätsring 1 1010 Wien.

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Onclick="window.open(this.href,'win2','status=no,toolbar=no,scrollbars=yes,titlebar=no,menubar=no,resizable=yes,width=640,height=480,directories=no,location=no'); return false;" rel="nofollow". Last Updated: 10 October 2016. How does protoplanetary disk gas and dust evolve, form water and organic molecules and transport them to the sites where habitable planets are forming? How does magnetic activity, the ionized wind, high-energy radiation and particles influence the planetary environment and interact w...

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